ASTROPHYSICAL S-FACTOR FOR O-16+O-16 WITHIN THE ADIABATIC MOLECULAR PICTURE

摘要

The astrophysical S-factor for O-16+O-16 is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the O-16+O-16 fusion cross section at deep sub-barrier energies.